Neutron Scattering - JUWEL - Forschungszentrum Jülich
Neutron Scattering - JUWEL - Forschungszentrum Jülich
Neutron Scattering - JUWEL - Forschungszentrum Jülich
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HEiDi 7<br />
The scattering factor F is a complex function describing the overlap of the scattering waves of<br />
each atom i (n per unit cell). si(Q) describes the scattering strength of the i-th atom on its<br />
position xi in dependence of the scattering vector Q, which depends on the character of cross<br />
section as described below.<br />
In this context one remark concerning statistics: For measurements of radiation the statistical<br />
error � is the square root of the number of measured events, e.g. x-ray or neutron particles.<br />
Thus, 100 events yield an error of 10% while 10,000 events yield an error of only 1%!<br />
Mean Square Displacements (MSD): Thermal movement of atoms around their average<br />
positions reduce the Bragg intensities during a diffraction experiment. The cause for this<br />
effect is the reduced probability density and therefore reduced cross section probability at the<br />
average positions. For higher temperatures (above a few Kelvin) the MSD Bi of the atoms<br />
increase linearly to the temperature T, this means B ~ T. Near a temperature of 0 K the MSD<br />
become constant with values larger than zero (zero point oscillation of the quantum<br />
mechanical harmonic oscillator).<br />
Thus, the true scattering capability si of the i-th atom in a structure has to be corrected by an<br />
angle-dependent factor (the so called Debye-Waller factor):<br />
si(Q) � si(Q) * exp(-Bi(sin �Q/�) 2 )<br />
This Debye-Waller factor decreases with increasing temperatures and yields an attenuation of<br />
the Bragg reflection intensities. At the same time this factor becomes significantly smaller<br />
with larger sin���~|Q|. Therefore, especially reflections with large indices loose a lot of<br />
intensity. The formula for anisotropic oscillations around their average positions looks like<br />
this:<br />
si(Q) � si(Q) * exp(-2� 2 (U i 11 h 2 a* 2 + U i 22 k 2 b* 2 + U i 33 l 2 c* 2 +<br />
+ 2U i 13 hl a*c* + 2U i 12 hk a*b* + 2U i 23kl b*c*))<br />
The transformation between B and Ueq (from the Uij calculated isotropic MSD for a sphere<br />
with identical volume) yields B = 8� 2 Ueq.<br />
For some structures the experimentally determined MSD are significantly larger than from the<br />
harmonic calculations of the thermal movement of the atoms expected. Such deviations can<br />
have different reasons: Static local deformations like point defects, mixed compounds,<br />
anharmonic oscillations or double well potentials where two energetically equal atomic<br />
positions are very near to each other and therefore distribute the same atom over the crystal<br />
with a 50%/50% chance to one or the other position. In all those cases an additional<br />
contribution to the pure Debye-Waller factor can be found which yields an increased MSD.<br />
Therefore in the following text only the term MSD will be used to avoid misunderstandings.<br />
3.2 Comparison of X-ray and <strong>Neutron</strong> Radiation<br />
X-Ray Radiation interacts as electromagnetic radiation only with the electron density in a<br />
crystal. This means the shell electrons of the atoms as well as the chemical binding. The<br />
scattering capability s (atomic form factor f(sin���)) of an atom depends on the number Z of<br />
its shell electrons (f(sin(�=0)/�) =Z). To be exact, f(sin(�)/�) is the Fourier transform of the<br />
radial electron density distribution ne(r): f(sin(�)/�)=s � � 0 4� 2 ne(r) sin(μr)/μr dr with<br />
μ=4�sin(�)/���Heavy atoms with many electrons contribute much stronger to reflection